Various gravitational, astrophysical and cosmological observations strongly imply the existence of Dark Matter (DM) in the universe. In particular, observations of the cosmological scale structure favour the so-called cold DM (CDM) scenario where the DM was not relativistic in the era of structure formation. In particle physics framework, the CDM scenario can be easily accounted for by extending the Standard Model (SM) with weakly interacting massive particles (WIMPs) – for a review see e.g. [1]} –. An interesting feature of the CDM scenario is that WIMPs with mass about \(\mathcal {O}(100)~\) GeV interacting primarily through weak interactions gives relic abundance of DM in agreement with the observation made by the Planck satellite, i.e. \(\Omega _{\mathrm {DM}} h^2 = 0.1188 \pm 0.0010\)  [2]}.
